The luminous eclipsing SMC OB + WN binary HD 5980 before and during the recent LBV-like outburst: An extreme case of colliding winds

The 1994 LBV-(luminous blue variable)like outburst of one of the luminous, hot components of the binary HD 5980 made it the brightest star in the Small Magellanic Cloud for an interval of 5 months. The most intriguing question to arise from this event is the following: Why did the HD 5980 spectrum c...

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Detalles Bibliográficos
Autores principales:	Moffat, A.F.J., Marchenko, S.V., Bartzakos, P., Nlemela, V.S., Cerruti, M.A., Magalhães, A.M., Balona, L., St-Louis, N., Seggewiss, W., Lamontagne, R.
Formato:	JOUR
Materias:	Stars: Binaries: Eclipsing Stars: Individual: HD 5980 Stars: Mass loss Stars: Variables Stars: Wolf-Ravet
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_0004637X_v497_n2PARTI_p896_Moffat
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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